后发座星系团(Coma Cluster of Galaxies)是现知最致密的星系团,它拥有数千个成员星系。NGC 4911就在这巨大星系团中心的 … xiaozhiya3.blog.163.com|基于20个网页 2. 后发星系团 coma是什么意思... ... 1.Coma cluster of galaxies后发星系团2. Having a coma;comate. 有种发的;多毛的 ... ...
This thesis will mainly focus on the lensing properties of N-body simulatedgalaxy clusters. 随后讨论了一个真实的N体数值模拟的星系团里的子结构和噪音对强引力透镜的影响。 更多例句>> 补充资料:后发星系团 后发星系团 Coma cluster of galaxies
(1971). Physical Sciences: X-rays from the Coma Cluster of Galaxies. Nature, 231:107-108.J. F. Meekins, G. Fritz, T. A. Chubb, and H. Friedman. Physical Sciences: X-rays from the Coma Cluster of Galaxies. Nature, 231:107-108, May 1971. doi: 10.1038/231107a0....
Clusters of galaxies are often embedded in larger-scale superclusters with dimensions of tens or perhaps even hundreds of Mpc. Observational and theoretical evidence suggest an important connection between cluster properties and their surroundings, with cluster formation being driven primarily by the in...
Coma clusternumber densitiesradial velocitiesHydra I ClusterPerseus Clusterclusters of galaxies/ A9850H Red shift, distances, and spatial distribution of galaxies A9850K Groups, clusters, and superclusters of galaxiesThe investigation of the distributions of number densities and radial velocities in the ...
galaxies: clusters: intracluster mediumgalaxies: evolutiongalaxies: kinematics and dynamicsintergalactic mediumWe present the results of deep imaging and spectroscopic observations of very extended ionized gas (EIG) around four member galaxies of the Coma cluster of galaxies: RB199, IC4040, GMP2923 and...
The Coma cluster of galaxies was observed with the position sensitive proportional counter (PSPC) during the ROSAT all sky survey. We find evidence for substructure in this cluster. Diffuse X-ray emission is detected from the regions of the NGC 4839 and 4911 subgroups at 6 percent and 1 perce...
Galaxy disruption as the origin of intracluster light in the Coma cluster of galaxies.Speculates on the cause of the large, low-surface brightness (LSD) features discovered in the Coma cluster of galaxies. Details on each of the LSB features; Interpretation; Production of linear features; ...
We present new measurements of the diffuse radio emission from the Coma cluster of galaxies at 1.4 GHz using the Effelsberg 100-m-telescope. The halo source Coma C has an extent down to noise of about 80 arcmin corresponding to 3 Mpc (H_0 = 50 km/s/Mpc) in Coma. The radio map ...
X-rays: galaxies: clustersThe brightest cluster radio halo known resides in the Coma cluster of galaxies. The relativistic electrons producing this diffuse synchrotron emission should also produce inverse Compton emission that becomes competitive with thermal emission from the intracluster medium (ICM) at...